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<ri:Resource created="2004-04-03T21:13:02Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Velocities of {lambda} Bootis stars</title><shortName>J/A+A/412/447</shortName><identifier>ivo://CDS.VizieR/J/A+A/412/447</identifier><altIdentifier>doi:10.26093/cds/vizier.34120447</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gerbaldi M.</name></creator><creator><name>Faraggiana R.</name></creator><creator><name>Lai O.</name></creator><date role="Updated">2017-09-22T16:16:24Z</date><date role="Created">2004-04-03T21:13:02Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>spectroscopic-binary-stars</subject><subject>variable-stars</subject><subject>radial-velocity</subject><description>We demonstrate that it is arduous to define the {lambda} Boo stars as a class of objects exhibiting uniform abundance peculiarities which would be generated by a mechanism altering the structure of their atmospheric layers. We collected the stars classified as {lambda} Boo up to now and discuss their properties, in particular the important percentage of confirmed binaries producing composite spectra (including our adaptive optics observations) and of misclassified objects. The unexplained RV variables (and thus suspected binaries), the known SB for which we lack information on the companion, the stars with an UV flux inconsistent with their classification, and the fast rotating stars for which no accurate abundance analysis can be performed, are also reviewed.</description><source format="bibcode">2003A&amp;A...412..447G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/412/447</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/V/50">V/50 : Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/381/105">J/A+A/381/105 : Rotational velocities of A-type stars. I. (Royer+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/393/897">J/A+A/393/897 : Rotational velocities of A-type stars II. 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